Infinite Curvature: Understanding Black Holes

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SUMMARY

The discussion centers on the concept of infinite curvature in relation to black holes, emphasizing that while black holes require significant mass to prevent light from escaping, infinite curvature is a theoretical construct that implies an infinitely massive object. The Riemann curvature tensor is identified as the fundamental tensor for measuring curvature in General Relativity (GR), with its components indicating the breakdown of the theory at singularities. The conversation highlights Einstein's perspective that space-time can bend but not rip, reinforcing the complexity of understanding black holes and their singularities.

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Familiarity with curvature tensors, specifically the Riemann curvature tensor
  • Basic knowledge of black hole physics
  • Conceptual grasp of space-time continuum
NEXT STEPS
  • Study the properties and implications of the Riemann curvature tensor in General Relativity
  • Explore the mathematical foundations of curvature in differential geometry
  • Investigate the nature of singularities in black hole physics
  • Review Einstein's theories on space-time and gravitational effects
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Astronomers, physicists, and students of theoretical physics who are interested in the complexities of black holes and the mathematical underpinnings of General Relativity.

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What does it mean for something to have an infinite curvature (like a black hole?)?
 
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Black holes do not necessarily have to have infinite curvature, but enough mass to prevent light from escaping its gravitational pull. Infinite curvature would require an infinitely massive object; it's only a theoretical idea and is probably not possible. Einstein didn't believe that space time could rip, but only bend.

If it could exist, it would mean that the space-time continuum was bent to infinity. In case you don't know, the space time continuum can be thought of as a soft surface (such as a mattress), that curves when a mass is on it, and that gives us the impression of gravitational acceleration. It’s a pretty “sketchy” way of thinking about it, but it works.
 
I checked for the definition of curvature, thinking I could come up with a good answer. I found many definitions of curvature! So I am leaving this one alone
 
In GR, curvature referes to one of several "curvatuare tensors". The most fundamental of these is the Riemann curvature tensor - if you know the values of the components of the Riemann curvature tensor, you can calculate the values of the other tensors (most notably the Ricci, Einstein, and perhaps the Weyl).

A tensor is not just a single number, but an "array" of related numbers.

"Infinite" means that the value of at least one of the components of said tensor (remember, a tensor is not just a single number) increases without bound as one approaches a point, such as the singularity of a black hole. This is usually taken to imply that the theory itself breaks down and is not valid at that singular point.

unfortunately, there isn't any really super-simple way to describe what the Riemann curvature measures, though this is discussed in, for instance:

http://math.ucr.edu/home/baez/gr/outline2.html
http://math.ucr.edu/home/baez/einstein/node9.html
 
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